利用高精度加速度计数据监测 JUICE 部署运行情况

IF 3.1 2区 物理与天体物理 Q1 ENGINEERING, AEROSPACE Acta Astronautica Pub Date : 2024-09-23 DOI:10.1016/j.actaastro.2024.09.047
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引用次数: 0

摘要

木星冰月探测器(JUICE)任务是欧空局2015-2025年宇宙愿景计划的基石,该计划致力于对木星及其冰月进行科学探索。JUICE于2023年4月14日从法属圭亚那发射升空,它将执行多重重力辅助,包括前所未有的月地双重重力辅助,以确定其飞往木星的轨道,并于2031年7月抵达木星。借助 10 套科学仪器,JUICE 将对木星系统进行全面调查,重点是木卫三。这些实验包括木星和伽利略卫星的重力和地球物理学(3GM)无线电科学和行星大地测量实验,由星载高精度加速计(HAA)提供支持。HAA 是一个三轴弹簧质量加速度计,用于测量作用在航天器上的非重力扰动,为了充分利用 3GM 的高精度测距和测距速率测量,需要对这些扰动进行测量。本文分析了在任务早期阶段收集的 HAA 数据,以监测航天器移动附属装置的初始部署。在附属装置的部署过程中,磁强计吊杆和太阳能电池阵列的振动模式以及朗缪尔探针铰链的锁定都被清晰地探测到。检测到的第一和第二磁强计吊杆弯曲模式的共振频率分别为 0.44 和 0.46 赫兹。HAA 数据有助于确定冰月探测雷达(RIME)天线部署异常的根本原因。致动器启动时产生的强烈外部扰动被用来描述航天器静止时间的特征。尽管在部署过程中航天器本底噪声明显增加,但仪器在 10 分钟内就恢复了全部灵敏度。这一信息可用于规划飞行任务科学阶段的航天器操作。
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Monitoring JUICE deployment operations with high-accuracy accelerometer data
The Jupiter Icy Moons Explorer (JUICE) mission is a cornerstone of ESA's Cosmic Vision 2015–2025 program devoted to the scientific exploration of Jupiter and its icy moons. Launched on April 14, 2023, from French Guiana, JUICE will perform multiple gravity assists, including an unprecedented lunar-Earth double gravity assist, in order to shape its trajectory to Jupiter, where it will arrive in July 2031. Thanks to a suite of 10 scientific instruments, JUICE will carry out a comprehensive investigation of the jovian system, with special focus on Ganymede. Among these experiments is the Gravity and Geophysics of Jupiter and the Galilean Moons (3GM) radio science and planetary geodesy experiment, supported by the onboard High Accuracy Accelerometer (HAA). The HAA, a three-axis spring mass accelerometer, measures the non-gravitational perturbations acting on the spacecraft, that need to be measured in order to fully exploit the highly accurate range and range rate measurements of 3GM. This paper analyzes the HAA data collected in the very early phase of the mission, to monitor the initial deployment of the spacecraft's moving appendages. The vibration modes of the magnetometer boom and solar arrays were clearly detected during the appendages' deployment, as well as the latching of the Langmuir probe hinges. The detected resonance frequencies of the first and second magnetometer boom bending modes are equal to 0.44 and 0.46 Hz, respectively. The HAA data contributed to identifying the root-cause of the anomalous Radar for Icy Moon Exploration (RIME) antenna deployment. The strong external perturbations due to the actuators' activation have been used to characterize the spacecraft tranquillization time. Despite the significant increase in the spacecraft noise floor during deployment events, the full sensitivity of the instrument was regained within 10 min. This information can be used to plan the spacecraft operations during the scientific phase of the mission.
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来源期刊
Acta Astronautica
Acta Astronautica 工程技术-工程:宇航
CiteScore
7.20
自引率
22.90%
发文量
599
审稿时长
53 days
期刊介绍: Acta Astronautica is sponsored by the International Academy of Astronautics. Content is based on original contributions in all fields of basic, engineering, life and social space sciences and of space technology related to: The peaceful scientific exploration of space, Its exploitation for human welfare and progress, Conception, design, development and operation of space-borne and Earth-based systems, In addition to regular issues, the journal publishes selected proceedings of the annual International Astronautical Congress (IAC), transactions of the IAA and special issues on topics of current interest, such as microgravity, space station technology, geostationary orbits, and space economics. Other subject areas include satellite technology, space transportation and communications, space energy, power and propulsion, astrodynamics, extraterrestrial intelligence and Earth observations.
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